UVCS MISSION LOG ---------------- Date: 29 July 2002 ----- Last revision: 05 August 2002 (Wu) -------------- File Name: 2002.07.30.a.log ----------- Compiled by: Y.-K. Ko ------------ UVCS Activity: Polar Coronal Hole Study for 30 - 31 July 2002 ------------ Mini-Synoptic for 31 July 2002 Polar Coronal Hole Study for 31 July 2002 SOHO Activity: -------------- EOF Staff: L. Zangrilli: Lead Scientist ---------- Y.-K. Ko: Commander, Planner M. Uzzo R. Wu Command file: 02.07.29.19:29:53.cmd.log Activity: --------- 1) Polar Coronal Hole Study Sequence: 02.07_lz1.tcl SCI_SPEC: To study the structure of newborn coronal holes of the new cycle, and to investigate a possible asymmetry between the north and the south poles. OBS_PROG: Primary: Spatial Coverage Sub Obj: Spectral Resolution SCI_OBJ: Primary: Coronal Structure Sub Obj: Large-Scale Structure OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2002.07.30.16:45 end: 2002.07.31.02:42 ONUMs = 17799 (114 exps) Instrument configuration: - Pointing: Sun center - Roll: 180 degrees (51551) - Mirror/Occulter: 1.6, 1.8, 2.0, 2.5, 3.0 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_LZ_194372 in Slot 4 Fits Files: q02.07.30.16:34:03.lya.dat q02.07.30.16:34:03.ovi.dat q02.07.30.16:34:03.vld.dat 2) Mini-Synoptic Sequence Load and Start Sequence: SynopticA:Mini SCI_SPEC: Synoptic studies. LYA HV off / OVI voltage at 210, LYA grating position now at 128000 "permanently". OBS_PROG: Synoptic SCI_OBJ: Synoptic OBJ: Entire Corona CMP_NAME: CMP_NUM: Duration: start: 2002.07.31.03:10 end: 2002.07.31.06:37 ONUMs = 39360 (9 exps) 39361 (9 exps) 39362 (9 exps) 39363 (9 exps) 39364 (9 exps) 39365 (8 exps) 39366 (9 exps) 39367 (9 exps) Instrument configuration: - Pointing: Sun center - Roll: W, NW, N, NE, E, SE, S, SW - Mirror/Occulter: 1.6, 1.75 Ro 1.5 mm overocculting (1.6 Ro) 2.0 mm overocculting (1.75 Ro) - LYA Slits: 50 um - OVI Slits: 150 um - LYA GRTPOS: 128000 - OVI GRTPOS: 173000 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_Syn3_173 in slot 2 Fits Files: z02.07.31.03:09:07.lya.dat z02.07.31.03:09:07.ovi.dat z02.07.31.03:09:07.vld.dat z02.07.31.03:35:47.lya.dat z02.07.31.03:35:47.ovi.dat z02.07.31.03:35:47.vld.dat z02.07.31.04:02:15.lya.dat z02.07.31.04:02:15.ovi.dat z02.07.31.04:02:15.vld.dat z02.07.31.04:28:44.lya.dat z02.07.31.04:28:44.ovi.dat z02.07.31.04:28:44.vld.dat z02.07.31.04:55:13.lya.dat z02.07.31.04:55:13.ovi.dat z02.07.31.04:55:13.vld.dat z02.07.31.05:21:57.lya.dat z02.07.31.05:21:57.ovi.dat z02.07.31.05:21:57.vld.dat GAP between 07/31/02|05:26:35( 8027) and 07/31/02|05:28:39( 8228) z02.07.31.05:48:34.lya.dat z02.07.31.05:48:34.ovi.dat z02.07.31.05:48:34.vld.dat z02.07.31.06:15:07.lya.dat z02.07.31.06:15:07.ovi.dat z02.07.31.06:15:07.vld.dat 3) Polar Coronal Hole Study Sequence: 02.07_lz2.tcl SCI_SPEC: To study the structure of newborn coronal holes of the new cycle, and to investigate a possible asymmetry between the north and the south poles. OBS_PROG: Primary: Spatial Coverage Sub Obj: Spectral Resolution SCI_OBJ: Primary: Coronal Structure Sub Obj: Large-Scale Structure OBJ: Coronal Hole CMP_NAME: CMP_NUM: Duration: start: 2002.07.31.06:44 end: 2002.07.31.16:41 ONUMs = 17800 (113 exps) Instrument configuration: - Pointing: Sun center - Roll: 180 degrees (51551) - Mirror/Occulter: 3.0, 3.5 Ro 1.5 mm overocculting - LYA Slit: 50 um - OVI Slit: 100 um - LYA GRTPOS: 128000 - OVI GRTPOS: 194372 - LYA mask: LYA_93_1sec in slot 2 - OVI mask: OVI_LZ_194372 in Slot 4 Fits Files: q02.07.31.06:37:53.lya.dat q02.07.31.06:37:53.ovi.dat q02.07.31.06:37:53.vld.dat